Titlebook: Relativity and Gravitation; 100 Years after Eins Ji?í Bi?ák,Tomá? Ledvinka Conference proceedings 2014 Springer International Publishing Sw

Intermediary

書目名稱Relativity and Gravitation影響因子(影響力)




書目名稱Relativity and Gravitation影響因子(影響力)學科排名




書目名稱Relativity and Gravitation網(wǎng)絡公開度




書目名稱Relativity and Gravitation網(wǎng)絡公開度學科排名




書目名稱Relativity and Gravitation被引頻次




書目名稱Relativity and Gravitation被引頻次學科排名




書目名稱Relativity and Gravitation年度引用




書目名稱Relativity and Gravitation年度引用學科排名




書目名稱Relativity and Gravitation讀者反饋




書目名稱Relativity and Gravitation讀者反饋學科排名

Uncultured

Black Hole Formation from a Complete Past for the Einstein–Vlasov System contains a black hole. In [.] initial data of this kind is constructed for the spherically symmetric Einstein–Vlasov system. One consequence of the result is that there exists a class of initial data for which the ratio of the Hawking mass . and the area radius . is arbitrarily small everywhere, su

amnesia

flaunt

Hidden Symmetries of the Dirac Equation in Curved Space-Timegeneral results on the relation between special spacetime tensors and hidden symmetries, both for the full Dirac equation and for its semi-classical limit, the spinning particle. A concrete application of the general results is provided by the case of rotating higher dimensional black holes with cos

Wordlist

Geometrostatics: The Geometry of Static Space-Times setup, we introduce localized formulas for the ADM-mass and ADM/CMC-center of mass of geometrostatic systems. We then explain the pseudo-Newtonian character of these formulas and show that they converge to Newtonian mass and center of mass in the Newtonian limit, respectively, using Ehlers’ frame t

abreast

The Gravitational Equation in Higher Dimensionsion of motion, it is possible to define a specific homogeneous polynomial analogue of the Riemann curvature, and then the trace of its Bianchi derivative yields the corresponding polynomial analogue of the divergence free Einstein tensor defining the differential operator for the equation of motion.

思想上升

accomplishment

Scalar Fields on Anti-de Sitter Backgroundti-de Sitter spacetime. In this short paper we consider the question how different the scalar field evolution is when the background is a fixed AdS metric. It is known that self-interacting massive real scalar fields on flat Minkowski background can form long living oscillating localized objects, na

欺騙世家

Einstein’s “Prague Field Equation” of 1912: Another Perspectivetion follows from the self-consistent implementation of the principle that . forms of energy are the source of the gravitational field according to .. This makes it an interesting toy-model for the “flat-space approach” to General Relativity (GR), as pioneered by Kraichnan and later Feynman. Solutio

Minutes